Motivated by Andy Weir's novel Hail Mary, I was just reading an answer regarding the time needed to travel between stars with a constant acceleration (and deceleration after the mid-way point). Due to time and space dilation, travel times become surprisingly short: For example, traveling to Kepler 186f that is 490 light years away would only take subjective 12.1 years. Since nothing can travel faster than light this implies that due to space dilation, the star must be much closer in the ship's reference frame at maximum speed; by necessity, closer than 12.1/2 light years. (I assume that because the ship is fastest at mid point, and the distance between Earth and star is shortest there, at maximum speed; the rest of the voyage is less efficient but the trip still takes no longer than 12.1 years. If the ship could continue to coast close to light speed from there (and then zoom by the star and not try to stay there), it would arrive much earlier than if it decelerated during the second half of the trip. Therefore, the star must be closer than 6.05 light years at that point, and the distance star-Sol would be < 12.1 light years.)
Now the star is, by observers on the ship, measured to be 490 light years away when the ship starts — but less than 12.1/2 at mid point. I suppose that is measured as the star (and everything else) moving by observers on that ship (and thus emitting blue-shifted light), just like we are seeing distant stars moving away from us in the expanding universe.
Didn't Kepler 186 just travel 472 or so light years in 6.05 years?